In science:

If the physical photon has signiﬁcant mixing with the trace U(1) photon, it seems likely therefore that a non-zero B ﬁeld would be felt as residual Lorentz violation rather than full blown noncommutative ﬁeld theory.

Noncommutativity from the string perspective: modification of gravity at a mm without mm sized extra dimensions

While the argument above was constructed for the toy model of Eq. (1), one could proceed identically for the full blown microscopic Hamiltonian of LiHoxY1−xF4 .

DC S = (0.482 ± 0.093)% This preliminary result preludes a full-blown lifetime analysis which soon will provide the FOCUS measurement of the r′ mixing parameter.

New FOCUS results on charm mixing and CP violation

An alternative approach is to undertake a full-blown Monte Carlo simulation of the most likely evolutionary scenarios described in §2.4.3.

Binary and Millisecond Pulsars at the New Millennium

Options considered ranged from simple rules and heuristic recipes, to extensive look-up tables using precomputed data, to full-blown “live” simulations of stellar and binary evolution and stellar hydrodynamics embedded in a dynamical code.

MODEST-1: Integrating Stellar Evolution and Stellar Dynamics

Somewhat fortuitously, ’low’, ’high’ and ’intermediate’ can also be taken to refer to BLN frequency (although in a full-blown HS the BLN is not detected).

A review of rapid X-ray variability in X-ray binaries

After all, the collective model of equation (5) was only the k = 0 part of the full blown Hamiltonian (1), but we did not consider the symmetry breaking ﬁeld to be only the k = 0 part of some other ﬁeld acting on all atoms individually.

Spontaneous Symmetry Breaking in Quantum Mechanics

The logic behind this deﬁnition of ¯G will be apparent later when we do a full-blown calculation of conductance.) The subscript on ¯G stands for the two states that are degenerate at this peak and the superscript reminds us that the Zeeman term is absent: EZ = 0.

Large spin-orbit effects in small quantum dots

This will provide tighter constraints for ΛCDM simulations that start from an inversion of the local density field, which routinely produce better galaxies than full-blown simulations.

Conference Summary: Magellanic System - Stars, Gas and Galaxies

Later on, we occasionally make a full-blown vortex detection, but only on the remaining basic particles, as the already detected vortexes are managed by the multiagent system.

Different goals in multiscale simulations and how to reach them

Studies of tensor models and GFT renormalization are just beginning, but already one example of a fully renormalizable non-trivial tensor model in 4 dimensions, though much simpler than full-blown GFTs for 4d gravity, has been recently exhibited .